Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Pakorn Wongwaitayakornkul"'
Fast magnetic reconnection involving non-MHD microscale physics is believed to underlie both solar eruptions and laboratory plasma current disruptions. While there is extensive research on both the MHD macroscale physics and the non-MHD microscale ph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bd42ba743e519dd0c98185433d05fb7
https://resolver.caltech.edu/CaltechAUTHORS:20200518-091931959
https://resolver.caltech.edu/CaltechAUTHORS:20200518-091931959
Autor:
Hui Li, Paul M. Bellan, Pakorn Wongwaitayakornkul, Byonghoon Seo, Magnus Haw, Ryan S. Marshall
Publikováno v:
Physics of Plasmas. 27:022109
We report the observations of a plasma jet evolving through a macro- to micro-scale progression sequence. This leads to a fast magnetic reconnection that results in the jet breaking off from its originating electrode and forming a force-free state. A
We report here a new model for explaining the three-part structure of coronal mass ejections (CMEs). The model proposes that the cavity in a CME forms because a rising electric current in the core prominence induces an oppositely directed electric cu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f49902e3aef563a5f2e847cbe9e826ef
https://resolver.caltech.edu/CaltechAUTHORS:20180801-103010822
https://resolver.caltech.edu/CaltechAUTHORS:20180801-103010822
We present a new theory for the presence of apex dips in certain experimental flux ropes. Previously such dips were thought to be projections of a helical loop axis generated by the kink instability. However, new evidence from experiments and simulat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b9cc17d95be0e9b4c4ecf2979c1945a
https://resolver.caltech.edu/CaltechAUTHORS:20171017-111654610
https://resolver.caltech.edu/CaltechAUTHORS:20171017-111654610
Publikováno v:
The Astrophysical Journal. 874:137
Single-pulse, globally propagating coronal fronts, called Extreme-ultraviolet (EUV) waves, were first observed in 1995 by the Extreme-ultraviolet Imaging Telescope and every observed EUV wave since has been associated with a coronal mass ejection (CM
Publikováno v:
Astrophysical Journal Letters; 2/1/2020, Vol. 889 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; Apr2019, Vol. 874 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal Letters; 8/1/2018, Vol. 862 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 10/20/2017, Vol. 848 Issue 2, p1-1, 1p